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<H3><A NAME="SECTION003432200000000000000">&#160;</A>
  <A NAME="irac2:alternative-construction">&#160;</A>
<BR>
Alternative construction
</H3>
  For a number of projects where very deep integrations and accurate
  flat fields are required, and the targets are point sources or much
  smaller than the frame size, the sky background itself can be used to
  calculate the flat field. When an object is dithered on the chip, so
  that it exposes pixels at different positions in different
  integrations, the resulting 'stack' of images may be combined to
  produce a very accurate flat field. Since a reference image, such as
  the ``LAMP OFF'' frame, is not subtracted, a bias frame of the same
  integration time must first be subtracted from all these images. They
  should then all be median combined, with suitable scaling introduced
  to match the medians of each image to account for the variability of
  the sky background level. The resulting image is then normalised to
  obtain the flat field.

<P>
To subtract the bias from the science images, use <TT>COMPUTE/IMAGE</TT>.
  Then use <TT>COMBINE/CCD</TT> to median all the frames
  together with multiplicative or additive scaling to match individual 
  frame medians (you should examine the results of both options to 
  determine which is working best for your data). Use <TT>STATISTICS/IMAGE</TT>
  to calculate the image median, and <TT>COMPUTE/IMAGE</TT> to divide by 
  this to get the normalised flat field.

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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
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